The concept of star multiplicity and its historical evolution

Details The concept of star multiplicity and its historical evolution The concept of star multiplicity and its historical evolution

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142...11f&link_type=abstract

(IAU, Colloquium on Wide Components in Double and Multiple Stars, 97th, Brussels, Belgium, June 8-13, 1987) Astrophysics and Spa

Astronomy and Astrophysics

Astrophysics

Binary Stars, Stellar Evolution, Stellar Systems, Radial Velocity, Stellar Spectrophotometry

Scientific paper

The history of the observation of double and multiple stars is reviewed, with emphasis on the impact of technical improvements in angular resolution, photometry, and radial velocity determination. Observational guidelines are discussed, and the need to investigate Selected Areas and the stars of Gliese's catalogue is pointed out. Future avenues of research include the systematic surveying of widely separated components, the adoption of trapezia and common proper motion stars within this family of objects, and the study of the photospheric phenomena of stars and their possible periodicity.

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